Photometry of a group of stars in the direction of NGC 1746/1750/1758
UBV broadband photometry is reported for 19 stars in the direction of the Galactic (open) star clusters NGC 1746/1750/1758. Nine of these stars possess proper motions that point to the existence of a group centered at α = 05h04m and δ = +23°43.5′. One known variable star, V1153 Tau, is recovered, and an emissionline star, HD 32318, is shown to be a variable star. RT Tau is reconfirmed to be constant in light. © 2010. The Astronomical Society of the Pacific. All rights reserved.
Publication Source (Journal or Book title)
Publications of the Astronomical Society of the Pacific
Landolt, A., & Africano, J. (2010). Photometry of a group of stars in the direction of NGC 1746/1750/1758. Publications of the Astronomical Society of the Pacific, 122 (895), 1008-1014. https://doi.org/10.1086/656322